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Quantum gravity Loop Quantum Gravity and Loop Quantum Cosmology Bjorn Solheim 04.05.2016 University of Oslo

Quantum gravity - Loop Quantum Gravity and Loop Quantum ... · Quantum gravity Loop Quantum Gravity and Loop Quantum Cosmology Bjorn Solheim 04.05.2016 University of Oslo. Contents

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Page 1: Quantum gravity - Loop Quantum Gravity and Loop Quantum ... · Quantum gravity Loop Quantum Gravity and Loop Quantum Cosmology Bjorn Solheim 04.05.2016 University of Oslo. Contents

Quantum gravity

Loop Quantum Gravity and Loop Quantum Cosmology

Bjorn Solheim

04.05.2016

University of Oslo

Page 2: Quantum gravity - Loop Quantum Gravity and Loop Quantum ... · Quantum gravity Loop Quantum Gravity and Loop Quantum Cosmology Bjorn Solheim 04.05.2016 University of Oslo. Contents

Contents

1. Introduction to the problem

of quantum gravity.

2. The theory of Loop quantum

gravity.

3. A simple Loop quantum

cosmology example

1

Page 3: Quantum gravity - Loop Quantum Gravity and Loop Quantum ... · Quantum gravity Loop Quantum Gravity and Loop Quantum Cosmology Bjorn Solheim 04.05.2016 University of Oslo. Contents

1. Introduction to quantum

gravity

Page 4: Quantum gravity - Loop Quantum Gravity and Loop Quantum ... · Quantum gravity Loop Quantum Gravity and Loop Quantum Cosmology Bjorn Solheim 04.05.2016 University of Oslo. Contents

Fundamental questions

What do space and time look

like on the very smallest scales?

What is space made of? Is there

such a thing as atoms of space?

Do space and time really exist,

or are they just emergent

concepts that serve as useful

approximations in some physical

domains?

2

Page 5: Quantum gravity - Loop Quantum Gravity and Loop Quantum ... · Quantum gravity Loop Quantum Gravity and Loop Quantum Cosmology Bjorn Solheim 04.05.2016 University of Oslo. Contents

Microscopic Geometry

These are question about the microscopic structure of space and time.

To answer such question we need a theory of the structure of space and

time. So far our best such theory is General Relativity.

Let us look quickly about what GR tells us about the world.

3

Page 6: Quantum gravity - Loop Quantum Gravity and Loop Quantum ... · Quantum gravity Loop Quantum Gravity and Loop Quantum Cosmology Bjorn Solheim 04.05.2016 University of Oslo. Contents

Equivalence principle

The unique property of gravity is that it is a force that affects all matter

and energy in the same way. This property is summed up in the

equivalence principle.

The equivalence principle enables us to describe gravity as geometry.

GR describes gravity as spacetime curvature.

”Matter tells geometry how to curve. Geometry tells matter how to

move.”

4

Page 7: Quantum gravity - Loop Quantum Gravity and Loop Quantum ... · Quantum gravity Loop Quantum Gravity and Loop Quantum Cosmology Bjorn Solheim 04.05.2016 University of Oslo. Contents

Triple structure

The gravitational field in GR is a

field of momentous importance.

It gives a unified description of

several key aspects of nature:

1. The force of gravity

2. The metric and causal

structure of spacetime

3. The inertial structure of

space

5

Page 8: Quantum gravity - Loop Quantum Gravity and Loop Quantum ... · Quantum gravity Loop Quantum Gravity and Loop Quantum Cosmology Bjorn Solheim 04.05.2016 University of Oslo. Contents

A change of perspective

We need to fully embrace what

GR tell us about the true nature

of spacetime.

Newton was wrong. Spacetime

is not a separate entity.

There is no spacetime in itself –

spacetime IS the gravitational

field.

Inertia is not movement with

respect to some eternal

spacetime, but movement

relative to the gravitational field.

6

Page 9: Quantum gravity - Loop Quantum Gravity and Loop Quantum ... · Quantum gravity Loop Quantum Gravity and Loop Quantum Cosmology Bjorn Solheim 04.05.2016 University of Oslo. Contents

A change of perspective – Non-dynamic

We often view Minkowski spacetime as spacetime without gravity. This is

not helpful for the purpose of quantum gravity.

Minkowski spacetime is NOT spacetime without gravity. It is spacetime

where we can ignore the dynamic aspects of gravity.

7

Page 10: Quantum gravity - Loop Quantum Gravity and Loop Quantum ... · Quantum gravity Loop Quantum Gravity and Loop Quantum Cosmology Bjorn Solheim 04.05.2016 University of Oslo. Contents

A change of perspective – Nothingness

GR describes gravity as fields on

a differentiable manifold. A

differentiable manifold has no

metric.

The natural physical meaning of

a differentiable manifold is that

it represents pure nothingness. It

is a mathematical background,

representing non-existence.

8

Page 11: Quantum gravity - Loop Quantum Gravity and Loop Quantum ... · Quantum gravity Loop Quantum Gravity and Loop Quantum Cosmology Bjorn Solheim 04.05.2016 University of Oslo. Contents

A change of perspective – Start with nothing

Instead of regarding Minkowski space as perhaps the ”default state” of

GR. It is more useful for our purposes today to consider the default or

basic state of GR to be a differentiable manifold without a metric. That

is, no spacetime at all, only the non-physical mathematical emptiness.

”In the beginning the world was an empty void without form. Then,...

GOD created the gravitational field, and there was space, and time and

spacetime, and all was right with the world.”

9

Page 12: Quantum gravity - Loop Quantum Gravity and Loop Quantum ... · Quantum gravity Loop Quantum Gravity and Loop Quantum Cosmology Bjorn Solheim 04.05.2016 University of Oslo. Contents

Microscopic geometry

GR is very successful, but as a purely classical theory can it describe

microscopic geometry?

What does other theories of the microscopic domain tell us?

10

Page 13: Quantum gravity - Loop Quantum Gravity and Loop Quantum ... · Quantum gravity Loop Quantum Gravity and Loop Quantum Cosmology Bjorn Solheim 04.05.2016 University of Oslo. Contents

Microscopic geometry

All other forces are described by

quantum theories not classical

theories.

This suggests that to answer

question about microscopic

geometry we need a quantum

theory of geometry.

Can we apply QFT insights to

GR?

11

Page 14: Quantum gravity - Loop Quantum Gravity and Loop Quantum ... · Quantum gravity Loop Quantum Gravity and Loop Quantum Cosmology Bjorn Solheim 04.05.2016 University of Oslo. Contents

QFT vs GR

Possible conflict

Naively it is not so easy to combine GR and QFT. There seems to be

several potential conflicts between the foundations of GR and QFT.

QFT/SM says matter is a purely quantum phenomena, described by

operators and Hilbert space vectors, that lives on a smooth Minkowski

space with a fixed geometry, and evolves according to a global time

parameter.

GR says matter is described by a classical tensor field and lives on a

curved manifolds with a dynamic geometry with no global time

parameter available.

12

Page 15: Quantum gravity - Loop Quantum Gravity and Loop Quantum ... · Quantum gravity Loop Quantum Gravity and Loop Quantum Cosmology Bjorn Solheim 04.05.2016 University of Oslo. Contents

QFT vs GR

Figure 1: QFT vs GR

13

Page 16: Quantum gravity - Loop Quantum Gravity and Loop Quantum ... · Quantum gravity Loop Quantum Gravity and Loop Quantum Cosmology Bjorn Solheim 04.05.2016 University of Oslo. Contents

QFT vs GR

Empirical success

The spectacular phenomenological success of GR + SM/QFT has lead to

a long period in physics where the differences between GR and QFT have

been de-emphasized.

Although the underlying conflict between QFT and GR at the level of

principles is well known, this doesn’t always come to the surface, perhaps

because in practical applications they can be friends at a distance.

14

Page 17: Quantum gravity - Loop Quantum Gravity and Loop Quantum ... · Quantum gravity Loop Quantum Gravity and Loop Quantum Cosmology Bjorn Solheim 04.05.2016 University of Oslo. Contents

The official story – QFT and GR are friends (sort of!)

15

Page 18: Quantum gravity - Loop Quantum Gravity and Loop Quantum ... · Quantum gravity Loop Quantum Gravity and Loop Quantum Cosmology Bjorn Solheim 04.05.2016 University of Oslo. Contents

Large and small nicely separated

LARGE SMALL

Classical

+

dynamic

gravity

Quantum

+

static

gravity

Gravity

important

Gravity

NOT

important

Quantum

NOT

important

Quantum

important

Universe Planets Atoms LHC

16

Page 19: Quantum gravity - Loop Quantum Gravity and Loop Quantum ... · Quantum gravity Loop Quantum Gravity and Loop Quantum Cosmology Bjorn Solheim 04.05.2016 University of Oslo. Contents

You take that part...

17

Page 20: Quantum gravity - Loop Quantum Gravity and Loop Quantum ... · Quantum gravity Loop Quantum Gravity and Loop Quantum Cosmology Bjorn Solheim 04.05.2016 University of Oslo. Contents

...and I take this part

18

Page 21: Quantum gravity - Loop Quantum Gravity and Loop Quantum ... · Quantum gravity Loop Quantum Gravity and Loop Quantum Cosmology Bjorn Solheim 04.05.2016 University of Oslo. Contents

The truth?

19

Page 22: Quantum gravity - Loop Quantum Gravity and Loop Quantum ... · Quantum gravity Loop Quantum Gravity and Loop Quantum Cosmology Bjorn Solheim 04.05.2016 University of Oslo. Contents

No such separation!

LARGE SMALL X-SMALL

Classical

+

dynamic

gravity

Quantum

+

static

gravity

Quantum

+

dynamic

gravity

Gravity

important

Quantum

NOT

important

Quantum

& Gravity

important

Universe Planets Atoms LHC GUT Planck

=10−35m

20

Page 23: Quantum gravity - Loop Quantum Gravity and Loop Quantum ... · Quantum gravity Loop Quantum Gravity and Loop Quantum Cosmology Bjorn Solheim 04.05.2016 University of Oslo. Contents

Fundamental physics belongs in the X-small domain

LARGE SMALL X-SMALL

Classical

+

dynamic

gravity

Quantum

+

static

gravity

Quantum

+

dynamic

gravity

Gravity

important

Quantum

NOT

important

Quantum

& Gravity

important

Universe Planets Atoms LHC GUT Planck

= 10−35m

21

Page 24: Quantum gravity - Loop Quantum Gravity and Loop Quantum ... · Quantum gravity Loop Quantum Gravity and Loop Quantum Cosmology Bjorn Solheim 04.05.2016 University of Oslo. Contents

Conceptual failure

Empirical success, conceptual failure

QFT (as formulated for the SM) depends crucially on features of

spacetime which GR tell us only applies in limited domains.

GR depends on features of matter which SM tells us is only true as a

large scale approximation.

The peaceful coexistence of SM and GR is an illusion stemming from the

fact that we live in a very big universe with very light fundamental

particles.

22

Page 25: Quantum gravity - Loop Quantum Gravity and Loop Quantum ... · Quantum gravity Loop Quantum Gravity and Loop Quantum Cosmology Bjorn Solheim 04.05.2016 University of Oslo. Contents

Conceptual healing

Conceptual healing

We must look for a theory that is conceptually unified and internally

consistent (as well as being empirically correct).

Can we combine the principles of GR and QM in one theory?

And what would such a theory look like?

Can spacetime survive?

23

Page 26: Quantum gravity - Loop Quantum Gravity and Loop Quantum ... · Quantum gravity Loop Quantum Gravity and Loop Quantum Cosmology Bjorn Solheim 04.05.2016 University of Oslo. Contents

QFT vs GR – Core Principles

QFT

Basic structure

Noncommutative algebra

(operators)

States (Hilbert space)

Global time parameter

(Hamiltonian)

Geometry and symmetry

Fixed geometry

Global O(1,3) symmetry

Not DIFF invariant

GR

Basic structure

Commutative algebra

(functions)

States (Phase space)

No time parameter

(Hamiltonian vanishes)

Geometry and symmetry

No (prior) geometry

No isometries

DIFF invariant

24

Page 27: Quantum gravity - Loop Quantum Gravity and Loop Quantum ... · Quantum gravity Loop Quantum Gravity and Loop Quantum Cosmology Bjorn Solheim 04.05.2016 University of Oslo. Contents

Quantum theory + Dynamic geometry

QFT

Basic structure

Noncommutative algebra

(operators)

States (Hilbert space)Global time parameter

(Hamiltonian)

Geometry and symmetry

Fixed geometry

Global O(1,3) symmetry

Not DIFF invariant

GR

Basic structureCommutative algebra

(functions)

States (Phase space)

No time parameter

(Hamiltonian vanishes)

Geometry and symmetry

No (prior) geometry

No isometries

DIFF invariant

25

Page 28: Quantum gravity - Loop Quantum Gravity and Loop Quantum ... · Quantum gravity Loop Quantum Gravity and Loop Quantum Cosmology Bjorn Solheim 04.05.2016 University of Oslo. Contents

Quantum gravity – Challenges ahead

Methods

There are no known quantum gravity phenomena. Such phenomena likely

resides at the Planck scale way beyond current experimental reach. The

likelihood of getting decisive empirical input soon is small. Empirical

confirmation is of course still crucial to stay in the domain of science, but

it seems unlikely that experimental results will be the driving force of the

development of quantum gravity theories.

To make progress we have to rely on consistency, conceptual clarity,

enforcing the principles of known physics, and reproducing the empirical

success on known theories.

26

Page 29: Quantum gravity - Loop Quantum Gravity and Loop Quantum ... · Quantum gravity Loop Quantum Gravity and Loop Quantum Cosmology Bjorn Solheim 04.05.2016 University of Oslo. Contents

Quantum gravity – What do we need?

We need to build a theory with the following properties

Non-perturbative and Quantum

Background independent and Diff. invariant

Supports matter and geometric degrees of freedom

Does not depend on any time parameter

Space, time and spacetime emerge in the proper limit

27

Page 30: Quantum gravity - Loop Quantum Gravity and Loop Quantum ... · Quantum gravity Loop Quantum Gravity and Loop Quantum Cosmology Bjorn Solheim 04.05.2016 University of Oslo. Contents

2. Loop Quantum Gravity

Page 31: Quantum gravity - Loop Quantum Gravity and Loop Quantum ... · Quantum gravity Loop Quantum Gravity and Loop Quantum Cosmology Bjorn Solheim 04.05.2016 University of Oslo. Contents

Loop Quantum Gravity

Loop Quantum Gravity (for the purposes of this talk) is a canonical

quantization of a gauge theory formulation of GR, with the connection as

the fundamental variable instead of the metric.

28

Page 32: Quantum gravity - Loop Quantum Gravity and Loop Quantum ... · Quantum gravity Loop Quantum Gravity and Loop Quantum Cosmology Bjorn Solheim 04.05.2016 University of Oslo. Contents

What is a constraint?

A constraint is a phase space function that we

require to be zero. This usually comes from

redundancies in the description of the system.

Let say we have a pendulum that is restricted to

swing in the xy-plane. If we choose to describe

the system by points in a three-dimensional

phase space (x , y , z) ∈ R3, we get two

constraint equations, x2 + y2 − L2 = 0 and

z = 0. These are not dynamical equations, they

just restrict the proper physical phase space to

a one-dimensional (3− 2 = 1) submanifold of

the original (redundant and un-physical)

three-dimensional manifold.

29

Page 33: Quantum gravity - Loop Quantum Gravity and Loop Quantum ... · Quantum gravity Loop Quantum Gravity and Loop Quantum Cosmology Bjorn Solheim 04.05.2016 University of Oslo. Contents

Dirac quantization of constrained systems

Full

Phase

Space

Physical

Phase

Space

Kinematical

Hilbert

Space

Physical

Hilbert

Space

Con

stra

ints

Quantization

Quantization

Con

stra

ints

30

Page 34: Quantum gravity - Loop Quantum Gravity and Loop Quantum ... · Quantum gravity Loop Quantum Gravity and Loop Quantum Cosmology Bjorn Solheim 04.05.2016 University of Oslo. Contents

Caution

Take a deep breath.. Heavy slide coming up.

31

Page 35: Quantum gravity - Loop Quantum Gravity and Loop Quantum ... · Quantum gravity Loop Quantum Gravity and Loop Quantum Cosmology Bjorn Solheim 04.05.2016 University of Oslo. Contents

The road to reality - Loop Quantum Gravity

1. Classical GR

2. SO(3)/SU(2)

Gauge theory

H = λiGi + NaDa + NH

3. Smear the variables to

get a Suitable sub-algebra.

The Holonomy-Flux algebra

a) Hamilt.

b) Diffeo.

c) Gauss

Constraints

4. HKin = Spin states

+ Quantum Algebra

5. Gauss constr.

HG = Spin-net. states

6. Diffeomorph. constr.

HDiff = Knot states

7. Hamiltonian constr.

HPhys = Physical states

8. Fully constrained system.

No dynamical equations.

Use relational mechanics

to extract dynamics

9. Dynamical

Quantum

Geometry

10. Classical space, time and

spacetime emerges in the

N →∞ w/appropriate cond.

Quantization

H = 0, Da = 0G i = 0

G iΨ = 0

DaΨ = 0

HΨ = 0

32

Page 36: Quantum gravity - Loop Quantum Gravity and Loop Quantum ... · Quantum gravity Loop Quantum Gravity and Loop Quantum Cosmology Bjorn Solheim 04.05.2016 University of Oslo. Contents

Idea 1: GR as SO(3)/SU(2) Gauge theory

(gµν, gµν)(Aia,E

ai

)Rewrite as

SU(2) gauge theory

Replace the metric (and its derivative) by an SU(2) connection Aia and a

(densitized) triad field E ai .

Think of this as a standard SU(2) Yang-Mills theory (with some extra

constraint equations).

Note that we are now in the Hamiltonian field theory formulation. This

theory is defined on a three-dimensional (spatial) hypersurface Σ.

33

Page 37: Quantum gravity - Loop Quantum Gravity and Loop Quantum ... · Quantum gravity Loop Quantum Gravity and Loop Quantum Cosmology Bjorn Solheim 04.05.2016 University of Oslo. Contents

Idea 2: Smear the Gauge variables – Holonomy-Flux

(Aia,E

ai

)(g , g) ∈ SU(2)× su(2)

Smear along

edges and surfaces

The SU(2) connection is a one form and (the dual of) densitized triad is

a two form. We can integrate these variable along edges (1-D) and

surfaces (2-D ) (without using a metric!).

From this integration we get an SU(2) group element g (in the spin-J

representation) for each edge, and an su(2) algebra element g for each

surface.

34

Page 38: Quantum gravity - Loop Quantum Gravity and Loop Quantum ... · Quantum gravity Loop Quantum Gravity and Loop Quantum Cosmology Bjorn Solheim 04.05.2016 University of Oslo. Contents

Idea 2: Smear the Gauge variables – Holonomy-Flux

x

y

z

x

y

z

Holonomy

Edge e → g SU(2) element

e → he [A] = exp∫eAdλ = g ∈ SU(2)

Flux

Surface S → g su(2) element

S → FS [E ] =∫SEdS = g ∈ su(2)

35

Page 39: Quantum gravity - Loop Quantum Gravity and Loop Quantum ... · Quantum gravity Loop Quantum Gravity and Loop Quantum Cosmology Bjorn Solheim 04.05.2016 University of Oslo. Contents

Quantum excitations along the edges of an embedded graph.

x

y

z

For quantum states we only need to

focus on the configuration space. So

informally only ”half” of the phase space

we just described. The quantum states

are build from the basic excitations of

the connection field. In this case the

excitation are similar to Faraday lines of

the electric field. However in this case,

these are not excitations of some field

IN space, but excitations OF space

itself. The excitations goes along the

edges of an embedded graph.

36

Page 40: Quantum gravity - Loop Quantum Gravity and Loop Quantum ... · Quantum gravity Loop Quantum Gravity and Loop Quantum Cosmology Bjorn Solheim 04.05.2016 University of Oslo. Contents

Quantum states – Group elements on each edge

37

Page 41: Quantum gravity - Loop Quantum Gravity and Loop Quantum ... · Quantum gravity Loop Quantum Gravity and Loop Quantum Cosmology Bjorn Solheim 04.05.2016 University of Oslo. Contents

Quantum states – Group elements on each edge

38

Page 42: Quantum gravity - Loop Quantum Gravity and Loop Quantum ... · Quantum gravity Loop Quantum Gravity and Loop Quantum Cosmology Bjorn Solheim 04.05.2016 University of Oslo. Contents

Area is discrete

39

Page 43: Quantum gravity - Loop Quantum Gravity and Loop Quantum ... · Quantum gravity Loop Quantum Gravity and Loop Quantum Cosmology Bjorn Solheim 04.05.2016 University of Oslo. Contents

Space emerges in a limit

40

Page 44: Quantum gravity - Loop Quantum Gravity and Loop Quantum ... · Quantum gravity Loop Quantum Gravity and Loop Quantum Cosmology Bjorn Solheim 04.05.2016 University of Oslo. Contents

Problem of time – Relational mechanics

What is the problem of time in loop quantum gravity? The Hamiltonian

of the theory is a linear combination of constraints, and all (Dirac)

observables must commute with the constraints. Therefore the Dirac

observables must commute with the Hamiltonian. This means they do

not change under the flow generated by the Hamiltonian.

Superficially the observables are frozen in time and there is no change.

One can say that the ”time translations” generated by the Hamiltonian

are ”pure gauge”.

Several solution using relational mechanics exists. We will see an example

in the cosmology section.

41

Page 45: Quantum gravity - Loop Quantum Gravity and Loop Quantum ... · Quantum gravity Loop Quantum Gravity and Loop Quantum Cosmology Bjorn Solheim 04.05.2016 University of Oslo. Contents

3. Loop quantum cosmology

Page 46: Quantum gravity - Loop Quantum Gravity and Loop Quantum ... · Quantum gravity Loop Quantum Gravity and Loop Quantum Cosmology Bjorn Solheim 04.05.2016 University of Oslo. Contents

The road to reality - Loop Quantum Cosmology

1. Classical FLRW

k=0

2. Gauge theory

– constant on slice

a) Hamilt.

b) Diffeo.

c) Gauss

Constraints

3. Suitable sub-algebra

Holonomy-Flux

4. HKin = Alm. per. func.

+ Quantum Algebra

5. HGauge =

Automatic

6. HDiff =

Automatic

7. HPhys =

Difference equation

8. Loop

Quantum

Cosmology

Relational QM

Use φ as a clock

GΨ = 0

HaΨ = 0

HΨ = 0

Quantization

42

Page 47: Quantum gravity - Loop Quantum Gravity and Loop Quantum ... · Quantum gravity Loop Quantum Gravity and Loop Quantum Cosmology Bjorn Solheim 04.05.2016 University of Oslo. Contents

Loop quantum cosmology

We can now make an explicit expression of the Hamiltonian constraint.

Cgravity = Tr(hµi h

µj (hµi )−1(hµj )−1hµk

{(hµk )

−1,V})

= sin2(µc) [sin(µc)V cos((µc))− cos((µc)V sin(µc))]

This translates into the following difference equation

C−(v)Ψ(v − 4, φ) + C 0(v)Ψ(v , φ) + C+(v)Ψ(v + 4, φ) = 0

We add a homogenous scalar field to act as clock variable.

∂2φΨ(v , φ) = C−(v)Ψ(v − 4, φ) + C 0(v)Ψ(v , φ) + C+(v)Ψ(v + 4, φ)

43

Page 48: Quantum gravity - Loop Quantum Gravity and Loop Quantum ... · Quantum gravity Loop Quantum Gravity and Loop Quantum Cosmology Bjorn Solheim 04.05.2016 University of Oslo. Contents

Numerical solutions and effective equations

The Hamiltonian constraint can be solved numerically. We can also

develop effective equations to represent the dynamics. We shall only

present the effective Friedmann equation. The classical Friedmann

equation is given by (a

a

)2

=8πG

The modified effective equation is(a

a

)2

=8πG

(1− ρ

ρCrit

), ρCrit = 0.41ρPl

44

Page 49: Quantum gravity - Loop Quantum Gravity and Loop Quantum ... · Quantum gravity Loop Quantum Gravity and Loop Quantum Cosmology Bjorn Solheim 04.05.2016 University of Oslo. Contents

Quantum bounce

45

Page 50: Quantum gravity - Loop Quantum Gravity and Loop Quantum ... · Quantum gravity Loop Quantum Gravity and Loop Quantum Cosmology Bjorn Solheim 04.05.2016 University of Oslo. Contents

Quantum bounce

46

Page 51: Quantum gravity - Loop Quantum Gravity and Loop Quantum ... · Quantum gravity Loop Quantum Gravity and Loop Quantum Cosmology Bjorn Solheim 04.05.2016 University of Oslo. Contents

Quantum bounce, k = 1

47

Page 52: Quantum gravity - Loop Quantum Gravity and Loop Quantum ... · Quantum gravity Loop Quantum Gravity and Loop Quantum Cosmology Bjorn Solheim 04.05.2016 University of Oslo. Contents

Summary

Page 53: Quantum gravity - Loop Quantum Gravity and Loop Quantum ... · Quantum gravity Loop Quantum Gravity and Loop Quantum Cosmology Bjorn Solheim 04.05.2016 University of Oslo. Contents

Summary – Part I

Naively QFT + GR appears to separate nicely into small and big,

but this is an artifact of living in a big universe with very light

elementary particles.

The extra-small domain is the proper domain of fundamental

physics. No such separation exists there, and the current model is

inadequate.

Uniting QFT and GR likely requires developing some sort of

non-perturbative background independent quantum (field) theories.

Space, and time, and spacetime are all emergent phenomena and we

must use relational methods to define dynamics.

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Page 54: Quantum gravity - Loop Quantum Gravity and Loop Quantum ... · Quantum gravity Loop Quantum Gravity and Loop Quantum Cosmology Bjorn Solheim 04.05.2016 University of Oslo. Contents

Summary – Part II

LQG is a non-perturbative background independent quantization of

GR.

LQG implements the core principles of QM and GR.

LQG is mathematically rigorous and based on a clear set of ideas,

and results in a picture of space based on quantum geometry.

Time does not exist as a fundamental entity, and dynamics is

implemented by relational methods.

49

Page 55: Quantum gravity - Loop Quantum Gravity and Loop Quantum ... · Quantum gravity Loop Quantum Gravity and Loop Quantum Cosmology Bjorn Solheim 04.05.2016 University of Oslo. Contents

Summary – Part III

LQC is an application of LQG is simplified setting.

The quantum FLRW model eliminates the big bang singularity and

replaces it with a smooth bounce.

At super high density a very strong repulsive quantum geometric

force appears.

At lower density the model behaves the same as classical FLRW

cosmology

The model demonstrate the use of relational time and how smooth

spacetime emerges from the quantum geometric picture.

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Page 56: Quantum gravity - Loop Quantum Gravity and Loop Quantum ... · Quantum gravity Loop Quantum Gravity and Loop Quantum Cosmology Bjorn Solheim 04.05.2016 University of Oslo. Contents

Extra Material

Page 57: Quantum gravity - Loop Quantum Gravity and Loop Quantum ... · Quantum gravity Loop Quantum Gravity and Loop Quantum Cosmology Bjorn Solheim 04.05.2016 University of Oslo. Contents

Quantization

Symplectic manifold

Commutative

Poisson alg.

(C∞, {, }ω)

Classical

Suitable

subalgebra

αf

f + g

{f , g}ω

f ∗ g

Operator alg.

Non-Commutative

Poisson alg.

(B(H), [, ])

Quantum

Generalize

to full alg.

αF

F + G{F , G

}Q

= 1i~

[F , G

]

F ∗ G

Lie algebra

morphism

Deformation

51

Page 58: Quantum gravity - Loop Quantum Gravity and Loop Quantum ... · Quantum gravity Loop Quantum Gravity and Loop Quantum Cosmology Bjorn Solheim 04.05.2016 University of Oslo. Contents

Rewriting EH-action

Rewriting EH-action → hypersurface variables:

S =1

∫d4x√−gR

=1

∫dx0

∫d3x N

√q(R +

(qikqjl − qijqkl

)KijKkl)

Legendre transfromation:

Π =∂L

∂N= 0, Πa =

∂L

∂Na= 0,

Pab =∂L

∂qab=

1

κ

√q(qacqbd − qabqcd

)Kcd

The action becomes

S =1

∫dx0

∫d3x

{qabP

ab − [NaCa + NC ]}

52

Page 59: Quantum gravity - Loop Quantum Gravity and Loop Quantum ... · Quantum gravity Loop Quantum Gravity and Loop Quantum Cosmology Bjorn Solheim 04.05.2016 University of Oslo. Contents

First class constraints

We already saw two primary constraints coming directly from the

Legendre transformation

Π =∂L

∂N= 0, Πa =

∂L

∂Na= 0,

Preserving these two primary constraints under Hamiltonian (”time”)

evolution leads to two secondary constraints.

Π = C = 0, Πa = Ca = 0

C and Ca are called the Hamiltonian constraint and the diffeomorphism

constraint. The Hamiltonian is a linear combination of these constraints.

H =1

∫d3x {NaCa + NC}

53

Page 60: Quantum gravity - Loop Quantum Gravity and Loop Quantum ... · Quantum gravity Loop Quantum Gravity and Loop Quantum Cosmology Bjorn Solheim 04.05.2016 University of Oslo. Contents

Triads and Extrinsic curvature

We now exchange the metric for a set of triads (orthonormal frame

fields). The triads specify orthonormal basis in terms of the coordinate

basis.

~ei = eai ~ea, ~ea = e ia~ei

This gives

qab = ~ea · ~eb = e ia~ei · ejb~ej = e iae

jb (~ei · ~ej) = e iae

jb (δij)

The conjugate momenta of the triad is the extrinsic curvature with mixed

indices.

K ia = δabe jbKij

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Page 61: Quantum gravity - Loop Quantum Gravity and Loop Quantum ... · Quantum gravity Loop Quantum Gravity and Loop Quantum Cosmology Bjorn Solheim 04.05.2016 University of Oslo. Contents

Ashtekar variables

We move straight on to the final modification. Introducing the

Ashtekar-Barbero connection and the densitized triads. Notice the

arbitray Barbero-Immirzi parameter γ.

Aia := ωi

a + γK ia, E a

i :=√qeai

The Poisson brackets are simply{Aia(x),Aj

b(y)}

= 0,{E ai (x),E b

j (y)}

= 0,{Aia(x),E b

j (y)}

= γδij δba δ

3(x , y)

55

Page 62: Quantum gravity - Loop Quantum Gravity and Loop Quantum ... · Quantum gravity Loop Quantum Gravity and Loop Quantum Cosmology Bjorn Solheim 04.05.2016 University of Oslo. Contents

Holonomy-Flux

x

y

z

x

y

z

Holonomy

Edge e → g SU(2) element

e → he [A] = exp∫eAdλ = g ∈ SU(2)

Flux

Surface S → g su(2) element

S → FS [E ] =∫SEdS = g ∈ su(2)

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Page 63: Quantum gravity - Loop Quantum Gravity and Loop Quantum ... · Quantum gravity Loop Quantum Gravity and Loop Quantum Cosmology Bjorn Solheim 04.05.2016 University of Oslo. Contents

Holonomy-Flux

Figure 2: Holonomy line piercing a flux

surface.

The Poisson bracket of the

holonomies and the fluxes can

now be calculated. The Flux

splits the holonomy edge into

two holonomies and ”takes

down” a SU(2) generator at the

intersection point. In simplified

notation

{he [A] ,F} = he1 [A] τ ahe2 [A]

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Cylindrical functions

A (embedded) graph Γ is a

collection of edges ei inΣ.

Example Γ = {e1, e2}.

e1

e2

Σ

Phase space functions

f : A → C

Cylindrical functions

Depend on the connection only along

holonomy edges of a graph Γ.

Made by composition f = k ◦ h of a

holonomy map

hΓ : A → (he1 [A] , he2 [A])

and

k : SU(2)× SU(2)→ C

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Action on basis states

Action of SU(2) gauge constraint. A gauge transformation on Σ is given

by a map θ : Σ→ G . The effect of such a transformation on a holonomy

is given by

he [A]→ θ(e0)he [A] θ(e1).

Action of a diffeomorphism φ : Σ→ Σ on a holonomy is

φhe [A] = hφ?e [A]

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Spin-network states – Evolution

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Constraints

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Physics: Area and Volume

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Idea 4: Use knots to make it DIFF invariant.

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